Description | Resolving Vela pulsars emission region directly via scintellometry |
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Antennas | Pa-At-Ho-Cd-Ti-Ak |
Start | 64 06:00:00 |
Stop | 64 10:30:00 |
PI | Jean-Pierre Macquart |
Setup lba18cm-2p-2IF:
Station Modes | Pa At Ho Cd |
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Channel 1 | IFP#1-LO 1634 - 1650 MHz USB RCP |
Channel 2 | IFP#1-HI 1650 - 1666 MHz USB RCP |
Channel 3 | IFP#2-LO 1634 - 1650 MHz USB LCP |
Channel 4 | IFP#2-HI 1650 - 1666 MHz USB LCP |
DAS 1 Skyfreq | 1650 MHz |
Bandwidth | 16 MHz |
DAS Mode | vsop.pro (telescope) |
Station Modes | Ti |
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Channel 1 | IFP#1-LO 1634 - 1650 MHz USB LCP |
Channel 2 | IFP#1-HI 1650 - 1666 MHz USB LCP |
DAS 1 Skyfreq | 1650 MHz |
Bandwidth | 16 MHz |
DAS Mode | vsop.pro (telescope) |
Station Modes | Ak |
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Channel 1 | IFP#1 1618 - 1682 MHz USB RCP |
Channel 2 | IFP#2 1618 - 1682 MHz USB LCP |
DAS 1 Skyfreq | 1650 MHz |
Bandwidth | 64 MHz |
DAS Mode | 64MHz_[nf].pro (telescope) |
Ftp: ftp://ftp.atnf.csiro.au/pub/people/vlbi/v537/v537a
Pulsar observation: please disable AGC in DAS, continuous noise cal, and PCAL where applicable.
ATCA antenna summary
Parkes onsource flagging
ATCA onsource flagging
Mopra onsource flagging
Mopra Tsys
(plot)
Parkes Tsys